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Fig. 1.

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MWL light curves covering the time period from November 5, 2009, (MJD 55140) to July 3, 2010, (MJD 55380). Top to bottom: MAGIC fluxes in daily bins for two energy bands (note the two different y-axes); VHE fluxes obtained from MAGIC and VERITAS above 0.2 TeV (in log scale); Fermi-LAT fluxes in 3-day bins in two energy bands; X-ray fluxes in 1-day bins from the all-sky monitors Swift-BAT and RXTE-ASM; X-ray fluxes from the pointing instruments Swift-XRT and RXTE-PCA; hardness ratio between the high and low-energy fluxes of Swift-XRT and between the two VHE bands of MAGIC (note the two different y-axes); optical R-band data from GASP-WEBT; radio data from Metsähovi, UMRAO, SMA, OVRO and VLBA; polarization degree and polarization angle observations in the optical from the Steward and Perkins observatories and in radio from VLBA.

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